We propose that a gamma-ray burst in one member of a binary may induce a su
pernova-like explosion of a close, white dwarf companion. Such an explosion
might be brought about in rather light companions, which cannot undergo th
e standard accretion-induced explosion. This would give some supernovae ass
ociated with gamma-ray bursts an appearance rather unlike that of the typic
al Type I supernova. GRB 980425, if indeed associated with SN 1998bw, is to
o weak to have produced the latter through our proposed mechanism.